We analyze archival ROSAT data of the CrA star forming region. X-ray e
mission from five infrared Class I protostars in the Coronet cluster w
as recently found in ASCA data, however, with low spatial resolution a
nd partly ambiguous source identification. ROSAT high spatial resoluti
on data confirm the X-ray detection of three Class I protostars. The o
ther two infrared protostars might be extincted to strongly for being
detected in the softer ROSAT bandpass. Alternatively, the X-ray emissi
on might be strongly variable and they might have been too faint in X-
rays at the time of the ROSAT observations.